Spectral determinations for discrete sources with EGRET

Details Spectral determinations for discrete sources with EGRET Spectral determinations for discrete sources with EGRET

May 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990nascp3071..201h&link_type=abstract

In NASA, Goddard Space Flight Center, The Energetic Gamma-Ray Experiment Telescope (EGRET) Science Symposium p 201-213 (SEE N90-

Physics

Crab Nebula, Energy Spectra, Gamma Rays, Parameter Identification, Point Sources, Spectrum Analysis, Gamma Ray Observatory, Gamma Ray Spectra, Gamma Ray Telescopes

Scientific paper

The ability of the EGRET (Energetic Gamma-Ray Experimental Telescope) to determine the spectral parameters of point sources in 14-day exposures, as planned for the initial survey phase of the GRO (Gamma Ray Observatory) mission, is explored by numerical simulation. Results are given for both galactic and extragalactic objects as a function of source strength and for representative levels of diffuse background emission.

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